Article contents
Mass–loss rates of cool evolved stars in M 33 galaxy
Published online by Cambridge University Press: 30 November 2022
Abstract
We have conducted a near-infrared monitoring campaign at the UK InfraRed Telescope (UKIRT), of the Local Group spiral galaxy M 33 (Triangulum). In this paper, we present the dust and gas mass-loss rates by the pulsating Asymptotic Giant Branch (AGB) stars and red supergiants (RSGs) across the stellar disc of M 33.
- Type
- Contributed Paper
- Information
- Proceedings of the International Astronomical Union , Volume 16 , Symposium S366: The Origin of Outflows in Evolved Stars , November 2020 , pp. 210 - 215
- Copyright
- © The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union
References
- 1
- Cited by